Open AccessEvidence for anomalous cloud particles at the poles of Venus
Author(s) -
Wilson C. F.,
Guerlet S.,
Irwin P. G. J.,
Tsang C. C. C.,
Taylor F. W.,
Carlson R. W.,
Drossart P.,
Piccioni G.
Publication year - 2008
Publication title -
journal of geophysical research: planets
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2008je003108
Subject(s) - venus , atmosphere of venus , radiative transfer , polar , polar vortex , physics , infrared , brightness , atmosphere (unit) , atmospheric sciences , latitude , astrophysics , astronomy , astrobiology , meteorology , optics
An analysis of near‐infrared emissions on the nightside of Venus observed by the Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) instrument on board Venus Express reveals anomalous cloud particles in the polar regions of Venus. These anomalous particles are found within the centers of polar vortices at both poles and are either larger or different in composition from those elsewhere in the planet. We find no persistent latitudinal variation in cloud properties at low to midlatitudes, nor do we find asymmetry between the southern and northern hemispheres. These findings arise from analysis of the relative brightness of 1.74 and 2.30 μ m infrared radiation thermally emitted from the deep atmosphere of Venus. Larger cloud particles cause relatively more attenuation at 2.30 μ m than at 1.74 μ m, so we use a “size parameter,” m = ( I 1.74 μ m )/( I 2.30 μ m ) 0.53 , as a proxy for particle size. This methodology follows that of Carlson et al. (1993), supported by new radiative transfer modeling.